Two Forms of Astrocyte Calcium Excitability Have Distinct Effects on NMDA Receptor-Mediated Slow Inward Currents in Pyramidal Neurons
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The Journal of Neuroscience, June 25, 2008 • 28(26):6659–6663 • 6659 Brief Communications Two Forms of Astrocyte Calcium Excitability Have Distinct Effects on NMDA Receptor-Mediated Slow Inward Currents in Pyramidal Neurons Eiji Shigetomi,1,2 David N. Bowser,3 Michael V. Sofroniew,2 and Baljit S. Khakh1,2,3 Departments of 1Physiology and 2Neurobiology, David Geffen School of Medicine, University of California, Los Angeles, California 90095-1751, and 3Medical Research Council Laboratory of Molecular Biology, Cambridge CB2 0QH, United Kingdom 2ϩ Astrocytes display excitability in the form of intracellular calcium concentration ([Ca ]i ) increases, but the signaling impact of these for 2ϩ neurons remains debated and controversial. A key unresolved issue is whether astrocyte [Ca ]i elevations impact neurons or not. Here we report that in the CA1 region of the hippocampus, agonists of native P2Y1 and PAR-1 receptors, which are preferentially expressed in 2ϩ astrocytes, equally elevated [Ca ]i levels without affecting the passive membrane properties of pyramidal neurons. However, under conditions chosen to isolate NMDA receptor responses, we found that activation of PAR-1 receptors led to the appearance of NMDA receptor-mediated slow inward currents (SICs) in pyramidal neurons. In stark contrast, activation of P2Y1 receptors was ineffective in 2ϩ this regard. The PAR-1 receptor-mediated increased SICs were abolished by several strategies that selectively impaired astrocyte [Ca ]i 2ϩ excitability and function. Our studies therefore indicate that evoked astrocyte [Ca ]i transients are not a binary signal for interactions with neurons, and that astrocytes result in neuronal NMDA receptor-mediated SICs only when appropriately excited. The data thus provide a basis to rationalize recent contradictory data on astrocyte–neuron interactions. Key words: astrocyte; calcium; SIC; gliotransmitter; astrocytic glutamate release; glia Introduction cellular Ca 2ϩ release (Newman, 2003a; Parri and Crunelli, 2003). 2ϩ Astrocytes, a type of glial cell, are found in the brain, and their Moreover, it is now well established that astrocyte [Ca ]i in- close spatial relationship to neurons is well documented (Araque creases trigger release of transmitters into the extracellular space. et al., 2001; Haydon, 2001). In addition to their important house- The evidence in favor of this is derived from a variety of ap- keeping roles (Kofuji and Newman, 2004), increasing evidence proaches, including biochemical, amperometric, and capacitance now suggests that astrocytes also actively participate in neuronal methods, as well as single-vesicle imaging (Araque et al., 2000; function (Haydon, 2001; Newman, 2003b; Fields, 2004; Fields Krzan et al., 2003; Bezzi et al., 2004; Evanko et al., 2004; Kreft et and Burnstock, 2006). al., 2004; Zhang et al., 2004a,b; Bowser and Khakh, 2007a; Jaiswal Astrocytes do not fire action potentials. However, they display et al., 2007). One of the transmitters known to be released from ϩ spontaneous and pharmacologically evoked intracellular Ca 2 astrocytes is glutamate. 2ϩ 2ϩ concentration ([Ca ]i) increases, which represent a form of as- The realization that astrocytes display [Ca ]i elevations and trocyte excitability. Since their initial discovery (Cornell-Bell et that they display calcium-triggered glutamate release raises the 2ϩ al., 1990) in astrocyte cultures, [Ca ]i increases have been ex- possibility that astrocytic glutamate could affect neurons. This tensively studied for in vitro preparations of brain slices (Haydon, issue has been addressed in the past, and we restrict ourselves here 2001; Parri et al., 2001; Newman, 2003b; Fields, 2004), and have to the most pertinent experiments for the CA1 region of the also been recorded from astrocytes in vivo with two-photon cal- hippocampus. In one study, NMDA receptor-mediated slow in- 2ϩ cium imaging from the cortex (Hirase et al., 2004). Thus [Ca ]i ward currents (SICs) were recorded from CA1 pyramidal neu- elevations appear to be a widespread and prevalent feature of rons when (S)-3,5-dihydroxyphenylglycine (DHPG) was used to astrocytes, can be triggered by neuronal activity, and are known activate metabotropic glutamate receptors on astrocytes and thus to occur independently of neuronal activity resulting from intra- 2ϩ trigger [Ca ]i elevations (Fellin et al., 2004). However, a recent study has questioned the use of DHPG because of its attendant Received April 20, 2008; revised May 15, 2008; accepted May 16, 2008. actions on neurons (Fiacco et al., 2007). Instead these authors This work was supported partly by the Medical Research Council, the Whitehall Foundation, and the Stein/ Oppenheimer Endowment Award (B.S.K.) and an Uehara Memorial Foundation Fellowship (Japan) (E.S.). used the creative approach of using an exogenous MrgA1 recep- 2ϩ Correspondence should be addressed to Baljit S. Khakh, Department of Physiology, University of California, Los tor selectively expressed in astrocytes to elevate [Ca ]i within Angeles, 10833 LeConte Avenue, 53-263 CHS, Los Angeles, CA 90095-1751. E-mail: [email protected]. 2ϩ them. They found that when astrocyte[Ca ]i levels were ele- D. N. Bowser’s present address: Howard Florey Institute, University of Melbourne, Parkville, Victoria 3010, vated by activating MrgA1 receptors, this did not result in the Australia. DOI:10.1523/JNEUROSCI.1717-08.2008 appearance of SICs in pyramidal neurons (Fiacco et al., 2007). Copyright © 2008 Society for Neuroscience 0270-6474/08/286659-05$15.00/0 Thus, the starkly contrasting conclusions between groups (Fellin 6660 • J. Neurosci., June 25, 2008 • 28(26):6659–6663 Shigetomi et al. • Astrocyte–Neuron Interactions et al., 2004; Fiacco et al., 2007) leaves open the question of 2ϩ whether astrocyte [Ca ]i elevations impact neurons or not (Tritsch and Bergles, 2007). In the present study, we returned to 2ϩ the issue of whether astrocyte [Ca ]i elevations can cause the appearance of SICs on pyramidal neurons. Materials and Methods Preparation of brain slices and electrophysiological recording. The methods used have been described previously (Khakh et al., 2003; Bowser and Khakh, 2004). Briefly, young [postnatal day 11 (P11)–P19] C57 mice were killed in accordance with institutional procedures. In some cases, GFAP-green fluorescent protein (GFP) mice were used, and these were available from previous work (Garcia et al., 2004). Coronal slices of hip- pocampus (200 or 300 m) were cut (model 1000 or 3000 Plus Vi- bratome) and submerged at room temperature in artificial CSF (aCSF) comprising the following (in mM): 126 NaCl, 2.5 KCl, 1.3 MgCl2,10 D-glucose, 2.4 CaCl2, 1.24 NaH2PO4, and 26 NaHCO3 saturated with 95% O2 and 5% CO2. Experiments were performed with potassium glu- conate or chloride-based internal solution, comprising the following (in Ϫ mM): 120 K gluconate (or Cl ), 10 KCl, 1 MgCl2, 0.03 CaCl2, 0.1 EGTA, 1 ATP, 0.2 GTP, 10 HEPES, and 4 glucose, pH 7.25. The resistance of the pipettes was ϳ4–9M⍀. Cells were visualized with infrared optics (Luigs and Neumann) on an upright microscope (Olympus BX50). We used bath application of agonists. Inward currents were recorded at Ϫ60 mV using pCLAMP 9 software, Multiclamp 900A amplifier, and Digidata 1322A (Molecular Devices). Spontaneous EPSCs were recorded in the presence of bicuculline (10 M) and D-(Ϫ)-2-amino-5-phosphono- pentanoic acid (D-AP5; 10 M). Slow inward currents (Fellin et al., 2004) mediated by extrasynaptic NMDA receptors were recorded in low-Mg 2ϩ buffers (0.13 mM) in the presence of bicuculline (10 M), TTX (1 M), and 6-cyano-2,3-dihydroxy-7-nitroquinoxaline (CNQX; 10 M). Astro- cytes were patched with 4–9 M⍀ electrodes filled with an intracellular solution comprising 123 CsCl, 1 MgSO , 10 HEPES, 1 ATP, 0.2 GTP, pH 4 2ϩ 7.35, and 100 M Alexa Fluor 488 (referred to as Alexa 488 in the text), Figure1. Astrocyte[Ca ]i transientsevokedbyactivationofP2Y1 andPAR-1receptors.A, M Representative images of the stratum radiatum region of the hippocampus with astrocytes and BAPTA (10 m ) as indicated in the text (Jourdain et al., 2007). ϩ 2ϩ 2 Confocal imaging of astrocyte Ca activity and dialysis. Brain slices showingincreasesin[Ca ]i duringactivationofPAR-1receptorswithTFLLRpeptide(30 M). were loaded at room temperature in the dark with 5 M Fluo-4 AM Arrowheads point to astrocytes showing intracellular calcium transients. B, Exemplar traces 2ϩ (Invitrogen) in aCSF for 60 min, then transferred to dye-free aCSF for at PAR-1- and P2Y1-evoked [Ca ]i transients. C, D, Pooled data for experiments such as those in least 30 min before experimentation to allow for cleavage of the AM ester A.Thegraylinesareindividualcells,andthesolidlinesaretheaveragesfromallcells.Activation 2ϩ group (Porter and McCarthy, 1996). Live astrocytes were predominantly of both P2Y1 and PAR-1 receptors evoked increases in astrocyte [Ca ]i levels. E, The average 2ϩ loaded with the fluorescent dye with these conditions. This was con- normalized traces for [Ca ]i transients evoked by P2Y1 and PAR-1 receptor activation; note firmed by simultaneous acquisition of infrared-differential interference that there was a latency for the PAR-1-mediated responses in relation to those mediated by contrast (IR-DIC) images of astrocytes in the same area. Cells and slices P2Y1 receptors, and their duration was longer. were imaged using an Olympus Fluoview 300 laser-scanning confocal microscope with a 300 mW argon laser, at Ͻ10% power. Emitted green fluorescence was collected through a 515 long-pass filter. Fluoview soft- vesicle exocytosis in culture (Bowser and Khakh, 2007a). PAR-1 ware was used for image acquisition. For BAPTA and Alexa 488 dialysis, receptors are known to be preferentially expressed within astro- the astrocytes were held at Ϫ80 mV, and depolarized to 0 mV for 100 ms cytes of the hippocampus (Weinstein et al., 1995; Junge et al., every 30 s to monitor access resistance. The optimal dialysis time was 2004; Lee et al., 2007). Thus, P2Y1 and PAR-1 receptors are useful empirically determined to be 15 min after patching.